The Giant Radio Array for Neutrino Detection (GRAND): Present and Perspectives
- Autores
- Fang, Ke; Alvarez Muñiz, Jaime; Alves Batista, Rafael; Bustamante, Mauricio; Carvalho Jr., Washington R.; Charrier, Didier; Cognard, Ismaël; de Jong, Sijbrand; De Vries, Krijn D.; Finley, Chad; Gou, Quanbu; Gu, Junhua; Guepin, Claire; Hanson, Jordan; Hu, Hongbo; Kotera, Kumiko; Le Coz, Sandra; Mao, Yi; Martineau Huynh, Olivier; Medina, Maria Clementina; Mostafa, Miguel; Mottez, Fabrice; Murase, Kohta; Niess, Valentin; Oikonomou, Foteini; Schröder, Frank G.; Tasse, Cyril; Timmermans, Charles; Renault Tinacci, Nicolas; Tueros, Matias Jorge; Wu, Xiang Ping; Zarka, Philippe; Zech, Andreas; Zhang, Yi; Zheng, Qian; Zilles, Anne
- Año de publicación
- 2017
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- The Giant Radio Array for Neutrino Detection (GRAND) aims at detecting ultra-high energy extraterrestrial neutrinos via the extensive air showers induced by the decay of tau leptons created in the interaction of neutrinos under the Earth?s surface. Consisting of an array of ∼ 1E5 radio antennas deployed over ∼ 2E5 km2, GRAND plans to reach, for the first time, an all-flavor sensitivity of ∼ 1.5E−10 GeV cm−2s−1 sr−1 above 5×1017 eV and a sub-degree angular resolution, beyond the reach of other planned detectors. We describe here preliminary designs and simulation results, plans for the ongoing, staged approach to the construction of GRAND, and the rich research program made possible by GRAND?s design sensitivity and angular resolution.
Fil: Fang, Ke. University of Maryland; Estados Unidos
Fil: Alvarez Muñiz, Jaime. Universidad de Santiago de Compostela. Facultad de Física; España
Fil: Alves Batista, Rafael. University of Oxford. Department of Physics; Reino Unido
Fil: Bustamante, Mauricio. Ohio State University; Estados Unidos
Fil: Carvalho Jr., Washington R.. Universidade de Sao Paulo; Brasil
Fil: Charrier, Didier. Universite de Nantes; Francia. Centre National de la Recherche Scientifique; Francia
Fil: Cognard, Ismaël. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia. Université d’Orléans; Francia
Fil: de Jong, Sijbrand. Radboud Universiteit Nijmegen. Instituto For Mathematics, Astrophysics And Particle Physics; Países Bajos
Fil: De Vries, Krijn D.. Vrije Unviversiteit Brussel; Bélgica
Fil: Finley, Chad. Stockholm University; Suecia
Fil: Gou, Quanbu. Chinese Academy of Sciences; República de China
Fil: Gu, Junhua. Chinese Academy of Sciences; República de China
Fil: Guepin, Claire. Sorbonne University; Francia
Fil: Hanson, Jordan. Ohio State University; Estados Unidos
Fil: Hu, Hongbo. Chinese Academy of Sciences; República de China
Fil: Kotera, Kumiko. Sorbonne University; Francia
Fil: Le Coz, Sandra. Chinese Academy of Sciences; República de China
Fil: Mao, Yi. Tsinghua University; China
Fil: Martineau Huynh, Olivier. Laboratoire de Physique Nucleaire Et de Hautes Energies; Francia. Universite de Paris VI; Francia. Université Paris Diderot - Paris 7; Francia
Fil: Medina, Maria Clementina. Laboratoire de Physique Nucleaire Et de Hautes Energies; Francia. Universite de Paris VI; Francia. Université Paris Diderot - Paris 7; Francia. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Mostafa, Miguel. State University Of Pennsylvania. Dept.of Physics; Estados Unidos. University Park; Estados Unidos
Fil: Mottez, Fabrice. Universite Blaise Pascal; Francia. Clermont Université; Francia
Fil: Murase, Kohta. State University Of Pennsylvania. Dept.of Physics; Estados Unidos. University Park; Estados Unidos
Fil: Niess, Valentin. Universite Blaise Pascal; Francia. Clermont Université; Francia
Fil: Oikonomou, Foteini. State University Of Pennsylvania. Dept.of Physics; Estados Unidos. University Park; Estados Unidos
Fil: Schröder, Frank G.. Karlsruher Institut Fur Technologie. Institut Fur Kernphysik; Alemania
Fil: Tasse, Cyril. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia. Université Paris Diderot - Paris 7; Francia. PSL Research University; Francia
Fil: Timmermans, Charles. Radboud Universiteit Nijmegen. Instituto For Mathematics, Astrophysics And Particle Physics; Países Bajos
Fil: Renault Tinacci, Nicolas. Institut Astrophysique de Paris; Francia. Sorbonne University; Francia
Fil: Tueros, Matias Jorge. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina
Fil: Wu, Xiang Ping. Chinese Academy of Sciences; República de China
Fil: Zarka, Philippe. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia
Fil: Zech, Andreas. Universite Blaise Pascal; Francia. Clermont Université; Francia
Fil: Zhang, Yi. Chinese Academy of Sciences; República de China
Fil: Zheng, Qian. Chinese Academy of Sciences; República de China
Fil: Zilles, Anne. Sorbonne University; Francia
35th International Cosmic Ray Conference
Busan
Corea del Sur
International Union of Pure and Applied Physics - Materia
-
Radio Detection
Extensive Air Showers
High Energy Cosmic Rays
High Energy Neutrinos - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/137972
Ver los metadatos del registro completo
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The Giant Radio Array for Neutrino Detection (GRAND): Present and PerspectivesFang, KeAlvarez Muñiz, JaimeAlves Batista, RafaelBustamante, MauricioCarvalho Jr., Washington R.Charrier, DidierCognard, Ismaëlde Jong, SijbrandDe Vries, Krijn D.Finley, ChadGou, QuanbuGu, JunhuaGuepin, ClaireHanson, JordanHu, HongboKotera, KumikoLe Coz, SandraMao, YiMartineau Huynh, OlivierMedina, Maria ClementinaMostafa, MiguelMottez, FabriceMurase, KohtaNiess, ValentinOikonomou, FoteiniSchröder, Frank G.Tasse, CyrilTimmermans, CharlesRenault Tinacci, NicolasTueros, Matias JorgeWu, Xiang PingZarka, PhilippeZech, AndreasZhang, YiZheng, QianZilles, AnneRadio DetectionExtensive Air ShowersHigh Energy Cosmic RaysHigh Energy Neutrinoshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The Giant Radio Array for Neutrino Detection (GRAND) aims at detecting ultra-high energy extraterrestrial neutrinos via the extensive air showers induced by the decay of tau leptons created in the interaction of neutrinos under the Earth?s surface. Consisting of an array of ∼ 1E5 radio antennas deployed over ∼ 2E5 km2, GRAND plans to reach, for the first time, an all-flavor sensitivity of ∼ 1.5E−10 GeV cm−2s−1 sr−1 above 5×1017 eV and a sub-degree angular resolution, beyond the reach of other planned detectors. We describe here preliminary designs and simulation results, plans for the ongoing, staged approach to the construction of GRAND, and the rich research program made possible by GRAND?s design sensitivity and angular resolution.Fil: Fang, Ke. University of Maryland; Estados UnidosFil: Alvarez Muñiz, Jaime. Universidad de Santiago de Compostela. Facultad de Física; EspañaFil: Alves Batista, Rafael. University of Oxford. Department of Physics; Reino UnidoFil: Bustamante, Mauricio. Ohio State University; Estados UnidosFil: Carvalho Jr., Washington R.. Universidade de Sao Paulo; BrasilFil: Charrier, Didier. Universite de Nantes; Francia. Centre National de la Recherche Scientifique; FranciaFil: Cognard, Ismaël. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia. Université d’Orléans; FranciaFil: de Jong, Sijbrand. Radboud Universiteit Nijmegen. Instituto For Mathematics, Astrophysics And Particle Physics; Países BajosFil: De Vries, Krijn D.. Vrije Unviversiteit Brussel; BélgicaFil: Finley, Chad. Stockholm University; SueciaFil: Gou, Quanbu. Chinese Academy of Sciences; República de ChinaFil: Gu, Junhua. Chinese Academy of Sciences; República de ChinaFil: Guepin, Claire. Sorbonne University; FranciaFil: Hanson, Jordan. Ohio State University; Estados UnidosFil: Hu, Hongbo. Chinese Academy of Sciences; República de ChinaFil: Kotera, Kumiko. Sorbonne University; FranciaFil: Le Coz, Sandra. Chinese Academy of Sciences; República de ChinaFil: Mao, Yi. Tsinghua University; ChinaFil: Martineau Huynh, Olivier. Laboratoire de Physique Nucleaire Et de Hautes Energies; Francia. Universite de Paris VI; Francia. Université Paris Diderot - Paris 7; FranciaFil: Medina, Maria Clementina. Laboratoire de Physique Nucleaire Et de Hautes Energies; Francia. Universite de Paris VI; Francia. Université Paris Diderot - Paris 7; Francia. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Mostafa, Miguel. State University Of Pennsylvania. Dept.of Physics; Estados Unidos. University Park; Estados UnidosFil: Mottez, Fabrice. Universite Blaise Pascal; Francia. Clermont Université; FranciaFil: Murase, Kohta. State University Of Pennsylvania. Dept.of Physics; Estados Unidos. University Park; Estados UnidosFil: Niess, Valentin. Universite Blaise Pascal; Francia. Clermont Université; FranciaFil: Oikonomou, Foteini. State University Of Pennsylvania. Dept.of Physics; Estados Unidos. University Park; Estados UnidosFil: Schröder, Frank G.. Karlsruher Institut Fur Technologie. Institut Fur Kernphysik; AlemaniaFil: Tasse, Cyril. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia. Université Paris Diderot - Paris 7; Francia. PSL Research University; FranciaFil: Timmermans, Charles. Radboud Universiteit Nijmegen. Instituto For Mathematics, Astrophysics And Particle Physics; Países BajosFil: Renault Tinacci, Nicolas. Institut Astrophysique de Paris; Francia. Sorbonne University; FranciaFil: Tueros, Matias Jorge. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; ArgentinaFil: Wu, Xiang Ping. Chinese Academy of Sciences; República de ChinaFil: Zarka, Philippe. Centre National de la Recherche Scientifique. Observatoire de Paris; FranciaFil: Zech, Andreas. Universite Blaise Pascal; Francia. Clermont Université; FranciaFil: Zhang, Yi. Chinese Academy of Sciences; República de ChinaFil: Zheng, Qian. Chinese Academy of Sciences; República de ChinaFil: Zilles, Anne. Sorbonne University; Francia35th International Cosmic Ray ConferenceBusanCorea del SurInternational Union of Pure and Applied PhysicsSissa2017info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectConferenciaJournalhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/137972The Giant Radio Array for Neutrino Detection (GRAND): Present and Perspectives; 35th International Cosmic Ray Conference; Busan; Corea del Sur; 2017; 1-91824-8039CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://pos.sissa.it/301/996/pdfinfo:eu-repo/semantics/altIdentifier/url/https://pos.sissa.it/301/info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1708.05128Internacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:04:11Zoai:ri.conicet.gov.ar:11336/137972instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:04:11.465CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
The Giant Radio Array for Neutrino Detection (GRAND): Present and Perspectives |
title |
The Giant Radio Array for Neutrino Detection (GRAND): Present and Perspectives |
spellingShingle |
The Giant Radio Array for Neutrino Detection (GRAND): Present and Perspectives Fang, Ke Radio Detection Extensive Air Showers High Energy Cosmic Rays High Energy Neutrinos |
title_short |
The Giant Radio Array for Neutrino Detection (GRAND): Present and Perspectives |
title_full |
The Giant Radio Array for Neutrino Detection (GRAND): Present and Perspectives |
title_fullStr |
The Giant Radio Array for Neutrino Detection (GRAND): Present and Perspectives |
title_full_unstemmed |
The Giant Radio Array for Neutrino Detection (GRAND): Present and Perspectives |
title_sort |
The Giant Radio Array for Neutrino Detection (GRAND): Present and Perspectives |
dc.creator.none.fl_str_mv |
Fang, Ke Alvarez Muñiz, Jaime Alves Batista, Rafael Bustamante, Mauricio Carvalho Jr., Washington R. Charrier, Didier Cognard, Ismaël de Jong, Sijbrand De Vries, Krijn D. Finley, Chad Gou, Quanbu Gu, Junhua Guepin, Claire Hanson, Jordan Hu, Hongbo Kotera, Kumiko Le Coz, Sandra Mao, Yi Martineau Huynh, Olivier Medina, Maria Clementina Mostafa, Miguel Mottez, Fabrice Murase, Kohta Niess, Valentin Oikonomou, Foteini Schröder, Frank G. Tasse, Cyril Timmermans, Charles Renault Tinacci, Nicolas Tueros, Matias Jorge Wu, Xiang Ping Zarka, Philippe Zech, Andreas Zhang, Yi Zheng, Qian Zilles, Anne |
author |
Fang, Ke |
author_facet |
Fang, Ke Alvarez Muñiz, Jaime Alves Batista, Rafael Bustamante, Mauricio Carvalho Jr., Washington R. Charrier, Didier Cognard, Ismaël de Jong, Sijbrand De Vries, Krijn D. Finley, Chad Gou, Quanbu Gu, Junhua Guepin, Claire Hanson, Jordan Hu, Hongbo Kotera, Kumiko Le Coz, Sandra Mao, Yi Martineau Huynh, Olivier Medina, Maria Clementina Mostafa, Miguel Mottez, Fabrice Murase, Kohta Niess, Valentin Oikonomou, Foteini Schröder, Frank G. Tasse, Cyril Timmermans, Charles Renault Tinacci, Nicolas Tueros, Matias Jorge Wu, Xiang Ping Zarka, Philippe Zech, Andreas Zhang, Yi Zheng, Qian Zilles, Anne |
author_role |
author |
author2 |
Alvarez Muñiz, Jaime Alves Batista, Rafael Bustamante, Mauricio Carvalho Jr., Washington R. Charrier, Didier Cognard, Ismaël de Jong, Sijbrand De Vries, Krijn D. Finley, Chad Gou, Quanbu Gu, Junhua Guepin, Claire Hanson, Jordan Hu, Hongbo Kotera, Kumiko Le Coz, Sandra Mao, Yi Martineau Huynh, Olivier Medina, Maria Clementina Mostafa, Miguel Mottez, Fabrice Murase, Kohta Niess, Valentin Oikonomou, Foteini Schröder, Frank G. Tasse, Cyril Timmermans, Charles Renault Tinacci, Nicolas Tueros, Matias Jorge Wu, Xiang Ping Zarka, Philippe Zech, Andreas Zhang, Yi Zheng, Qian Zilles, Anne |
author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
dc.subject.none.fl_str_mv |
Radio Detection Extensive Air Showers High Energy Cosmic Rays High Energy Neutrinos |
topic |
Radio Detection Extensive Air Showers High Energy Cosmic Rays High Energy Neutrinos |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
The Giant Radio Array for Neutrino Detection (GRAND) aims at detecting ultra-high energy extraterrestrial neutrinos via the extensive air showers induced by the decay of tau leptons created in the interaction of neutrinos under the Earth?s surface. Consisting of an array of ∼ 1E5 radio antennas deployed over ∼ 2E5 km2, GRAND plans to reach, for the first time, an all-flavor sensitivity of ∼ 1.5E−10 GeV cm−2s−1 sr−1 above 5×1017 eV and a sub-degree angular resolution, beyond the reach of other planned detectors. We describe here preliminary designs and simulation results, plans for the ongoing, staged approach to the construction of GRAND, and the rich research program made possible by GRAND?s design sensitivity and angular resolution. Fil: Fang, Ke. University of Maryland; Estados Unidos Fil: Alvarez Muñiz, Jaime. Universidad de Santiago de Compostela. Facultad de Física; España Fil: Alves Batista, Rafael. University of Oxford. Department of Physics; Reino Unido Fil: Bustamante, Mauricio. Ohio State University; Estados Unidos Fil: Carvalho Jr., Washington R.. Universidade de Sao Paulo; Brasil Fil: Charrier, Didier. Universite de Nantes; Francia. Centre National de la Recherche Scientifique; Francia Fil: Cognard, Ismaël. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia. Université d’Orléans; Francia Fil: de Jong, Sijbrand. Radboud Universiteit Nijmegen. Instituto For Mathematics, Astrophysics And Particle Physics; Países Bajos Fil: De Vries, Krijn D.. Vrije Unviversiteit Brussel; Bélgica Fil: Finley, Chad. Stockholm University; Suecia Fil: Gou, Quanbu. Chinese Academy of Sciences; República de China Fil: Gu, Junhua. Chinese Academy of Sciences; República de China Fil: Guepin, Claire. Sorbonne University; Francia Fil: Hanson, Jordan. Ohio State University; Estados Unidos Fil: Hu, Hongbo. Chinese Academy of Sciences; República de China Fil: Kotera, Kumiko. Sorbonne University; Francia Fil: Le Coz, Sandra. Chinese Academy of Sciences; República de China Fil: Mao, Yi. Tsinghua University; China Fil: Martineau Huynh, Olivier. Laboratoire de Physique Nucleaire Et de Hautes Energies; Francia. Universite de Paris VI; Francia. Université Paris Diderot - Paris 7; Francia Fil: Medina, Maria Clementina. Laboratoire de Physique Nucleaire Et de Hautes Energies; Francia. Universite de Paris VI; Francia. Université Paris Diderot - Paris 7; Francia. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina Fil: Mostafa, Miguel. State University Of Pennsylvania. Dept.of Physics; Estados Unidos. University Park; Estados Unidos Fil: Mottez, Fabrice. Universite Blaise Pascal; Francia. Clermont Université; Francia Fil: Murase, Kohta. State University Of Pennsylvania. Dept.of Physics; Estados Unidos. University Park; Estados Unidos Fil: Niess, Valentin. Universite Blaise Pascal; Francia. Clermont Université; Francia Fil: Oikonomou, Foteini. State University Of Pennsylvania. Dept.of Physics; Estados Unidos. University Park; Estados Unidos Fil: Schröder, Frank G.. Karlsruher Institut Fur Technologie. Institut Fur Kernphysik; Alemania Fil: Tasse, Cyril. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia. Université Paris Diderot - Paris 7; Francia. PSL Research University; Francia Fil: Timmermans, Charles. Radboud Universiteit Nijmegen. Instituto For Mathematics, Astrophysics And Particle Physics; Países Bajos Fil: Renault Tinacci, Nicolas. Institut Astrophysique de Paris; Francia. Sorbonne University; Francia Fil: Tueros, Matias Jorge. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina Fil: Wu, Xiang Ping. Chinese Academy of Sciences; República de China Fil: Zarka, Philippe. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia Fil: Zech, Andreas. Universite Blaise Pascal; Francia. Clermont Université; Francia Fil: Zhang, Yi. Chinese Academy of Sciences; República de China Fil: Zheng, Qian. Chinese Academy of Sciences; República de China Fil: Zilles, Anne. Sorbonne University; Francia 35th International Cosmic Ray Conference Busan Corea del Sur International Union of Pure and Applied Physics |
description |
The Giant Radio Array for Neutrino Detection (GRAND) aims at detecting ultra-high energy extraterrestrial neutrinos via the extensive air showers induced by the decay of tau leptons created in the interaction of neutrinos under the Earth?s surface. Consisting of an array of ∼ 1E5 radio antennas deployed over ∼ 2E5 km2, GRAND plans to reach, for the first time, an all-flavor sensitivity of ∼ 1.5E−10 GeV cm−2s−1 sr−1 above 5×1017 eV and a sub-degree angular resolution, beyond the reach of other planned detectors. We describe here preliminary designs and simulation results, plans for the ongoing, staged approach to the construction of GRAND, and the rich research program made possible by GRAND?s design sensitivity and angular resolution. |
publishDate |
2017 |
dc.date.none.fl_str_mv |
2017 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/publishedVersion info:eu-repo/semantics/conferenceObject Conferencia Journal http://purl.org/coar/resource_type/c_5794 info:ar-repo/semantics/documentoDeConferencia |
status_str |
publishedVersion |
format |
conferenceObject |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/137972 The Giant Radio Array for Neutrino Detection (GRAND): Present and Perspectives; 35th International Cosmic Ray Conference; Busan; Corea del Sur; 2017; 1-9 1824-8039 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/137972 |
identifier_str_mv |
The Giant Radio Array for Neutrino Detection (GRAND): Present and Perspectives; 35th International Cosmic Ray Conference; Busan; Corea del Sur; 2017; 1-9 1824-8039 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
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openAccess |
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